Asteroid
1024 Hale , provisional designation A923 YO13 , is a carbonaceous background asteroid from the outer regions of the asteroid belt , approximately 45 kilometers (28 miles) in diameter. The asteroid was discovered on 2 December 1923, by Belgian–American astronomer George Van Biesbroeck at the Yerkes Observatory in Wisconsin, United States.[ 1] It was named for American astronomer George Ellery Hale .[ 2] The dark C-type asteroid may have a rotation period of 16 hours.[ 4]
Orbit and classification
Hale is a non-family asteroid from the main belt's background population .[ 5] It orbits the Sun in the outer asteroid belt at a distance of 2.2–3.5 AU once every 4 years and 10 months (1,772 days; semi-major axis of 2.87 AU). Its orbit has an eccentricity of 0.22 and an inclination of 16° with respect to the ecliptic .[ 3] The body's observation arc begins at Yerkes Observatory with its first recorded observation in December 1928, or five years after its official discovery observation.[ 1]
Physical characteristics
Hale has been characterized as a carbonaceous C-type asteroid by Pan-STARRS' photometric survey and by the SDSS -MFB (Masi Foglia Binzel).[ 4] In the SMASS classification it is a "hydrated" Ch-subtype.[ 3]
Rotation period
In January 2013, a first rotational lightcurve of Hale was obtained from photometric observations by Michael S. Alkema at the Elephant Head Observatory (G35 ) in Arizona, United States. Analysis of the fragmentary lightcurve gave a rotation period of 16.0 hours with a brightness amplitude of 0.10 magnitude (U=1+ ).[ 13] As of 2018, no secure period has been obtained.[ 4]
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , Hale measures between 28.46 and 51.37 kilometers in diameter and its surface has an albedo between 0.0260 and 0.10.[ 6] [ 7] [ 8] [ 9] [ 10] [ 11] [ 12]
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0496 and a diameter of 41.28 kilometers based on an absolute magnitude of 10.8.[ 4]
Naming
This minor planet was named after George Ellery Hale (1868–1938), a prolific American astronomer and pioneer of a new generation of large aperture telescopes, namely the 60-inch Hale and the 100-inch Hooker telescope at Mount Wilson Observatory , as well as the 200-inch Hale telescope at Palomar Observatory . He founded the discovering Yerkes and Mount Wilson observatories and was their first director. Hale also founded The Astrophysical Journal and invented the spectroheliograph , which allowed to take monochromatic images of the Sun. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 98 ).[ 2]
References
^ a b c d "1024 Hale (A923 YO13)" . Minor Planet Center . Retrieved 16 March 2018 .
^ a b c Schmadel, Lutz D. (2007). "(1024) Hale". Dictionary of Minor Planet Names – (1024) Hale . Springer Berlin Heidelberg. p. 88. doi :10.1007/978-3-540-29925-7_1025 . ISBN 978-3-540-00238-3 .
^ a b c d e f "JPL Small-Body Database Browser: 1024 Hale (A923 YO13)" (2018-02-26 last obs.). Jet Propulsion Laboratory . Archived from the original on 6 August 2020. Retrieved 16 March 2018 .
^ a b c d e f g h i "LCDB Data for (1024) Hale" . Asteroid Lightcurve Database (LCDB). Retrieved 16 March 2018 .
^ a b "Asteroid 1024 Hale – Nesvorny HCM Asteroid Families V3.0" . Small Bodies Data Ferret . Retrieved 24 October 2019 .
^ a b c d Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos" . The Astronomical Journal . 152 (3): 12. arXiv :1606.08923 . Bibcode :2016AJ....152...63N . doi :10.3847/0004-6256/152/3/63 .
^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal . 791 (2): 11. arXiv :1406.6645 . Bibcode :2014ApJ...791..121M . doi :10.1088/0004-637X/791/2/121 . S2CID 119293330 .
^ a b c d Masiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017). "NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos" . The Astronomical Journal . 154 (4): 10. arXiv :1708.09504 . Bibcode :2017AJ....154..168M . doi :10.3847/1538-3881/aa89ec .
^ a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos" . The Astrophysical Journal . 814 (2): 13. arXiv :1509.02522 . Bibcode :2015ApJ...814..117N . doi :10.1088/0004-637X/814/2/117 . S2CID 9341381 . Retrieved 16 March 2018 .
^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal . 741 (2): 25. arXiv :1109.6407 . Bibcode :2011ApJ...741...90M . doi :10.1088/0004-637X/741/2/90 . S2CID 35447010 .
^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey" . Publications of the Astronomical Society of Japan . 63 (5): 1117– 1138. Bibcode :2011PASJ...63.1117U . doi :10.1093/pasj/63.5.1117 . (online , AcuA catalog p. 153 )
^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids" . The Astrophysical Journal Letters . 759 (1): 5. arXiv :1209.5794 . Bibcode :2012ApJ...759L...8M . doi :10.1088/2041-8205/759/1/L8 . S2CID 46350317 . Retrieved 16 March 2018 .
^ a b Alkema, Michael S. (July 2013). "Asteroid Lightcurve Analysis at Elephant Head Observatory: 2012 November - 2013 April" . The Minor Planet Bulletin . 40 (3): 133– 137. Bibcode :2013MPBu...40..133A . ISSN 1052-8091 . Retrieved 16 March 2018 .
^ a b Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results" . Icarus . 261 : 34– 47. arXiv :1506.00762 . Bibcode :2015Icar..261...34V . doi :10.1016/j.icarus.2015.08.007 . S2CID 53493339 . Retrieved 16 March 2018 .
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